1 / 7

Letter of intend for the Core programme

This document outlines the objectives and follow-up actions for the core programme focusing on data analysis related to exoplanet characterisation, including transit observations, eclipsing binaries, and the study of planetary systems. Specific teams such as LAM, Geneva, and German collaborative groups are involved in various aspects, including stellar parameter determination and physical processes impacting such observations. Key topics include rotation profiles, activity in giants, and atmospheric models, supported by advancements in statistical methods and non-linear modeling.

graham
Télécharger la présentation

Letter of intend for the Core programme

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Letter of intend for the Core programme * Exo 14 answers data analysis follow-up a few specific programmes * Sismo 34 answers, very inhomogeneous Data analysis, Stellar parameters global specific Physical processes Objects classes individuals

  2. Exoplanet programme - Characterisation of transits: Barge, LAM+ Rauer+Bouchy Moutou, LAM Deeg, +? Rouan, IDF group Ollivier IDF Team Rauer, german team + Deleuil, Barge Queloz, Geneve team+ - Follow-up: Deleuil, LAM+ Queloz+Rauer + Deeg+ Bouchy Queloz Bouchy photom: Rauer, german +Deleuil+Barge - Specific Ecclipsing binaries: Deeg+ Schneider Multiplanetary systems Erickson+ Rauer Atmospheric models Rauer+ german Tomography Fridlund+ Gondoin

  3. Sismo Data analysis Data analysis Time frequency Baudin Statistical weight: Kjedsen Non linear: Wuchterl

  4. Sismo:Stellar parameters and physical process Stellar parameters, evolution General proposals Modeling: Noels + Scuflaire Test evolution: Roxburgh + ? Stellar parameters determination: Michel, + very large Stellar parameters of solar like and intermediate: Monteiro+ Specific topics base of ZC solar like: Monteiro He ionisation zone solar like: Monteiro Superadiabatic laye solar like : Monteiro F and G pulsators Vauclair G Physical processes Driving mechanisms: Dupret LESIA+ Garrido+belges+ Groghacene Excitation and damping: Samadi LESIA + baudin+ Rotation inversion Abundance stratification

  5. Sismo AcroCoRot, AcroCoRoT Momentum transport: Goupil Rotation profiles: Monteiro Rotation and fundamental parameters F and G Vauclairg Microvariability( G,K,M): Aigrain Solar-like activity: Foing + Aigrain+ lanza Conv and activity in giants: Gondoin+ fridlund+ Goupil… Accoustic background roca cortes Rotation period, diff rotation: Hatzes Magnetic field: Monteiro + APs

  6. Objects Objects: classes - Hot stars: presupernovae: Aerts+Team - B without emission:Aerts+Team - Be Hubert+ Be team - Red giants: Barban, Weiss + Team - Gamma dor: Mathias+ Team - Ap versus A Monteiro - Am: Vauclair S. - Delta scuti: Roca Cortes - Solar like main sequence: Roca Cortes - With and without planets: Monteiro - Ecclipsing binaries: Roca Cortes + APs Individuals: - HD 52265 Vauclair G (2?) - HD 50747 and 51106 (Am) Vauclair, S. - HD 50890 (red gaint) Vauclair G.

  7. Actions… * Meetings before launch on some topics Acrocorot Solar like * Answer to the letters ……..

More Related